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Structure of the lunar mantleThe structure of the lunar mantle is examined by using data on the decay of shear wave amplitude with distance and the relative arrival times of P and S waves. The new analysis confirms a previous lunar model based primarily upon travel times and more closely defines certain properties of the lunar mantle. A negative shear wave velocity gradient of 0.0013 (km/s)/km, shear wave Q of 4000, and Poisson's ratio of 0.250 plus or minus 0.025 are found for the upper mantle, which lies between the depths of 60 and 300 km. A rapid decrease of shear wave velocity with increasing depth is observed starting at around a 300-km depth, associated with a lower Q for shear waves. Poisson's ratio in the lower part of the middle mantle, which extends to a depth of about 1000 km, is estimated to be 0.36 plus or minus 0.02.
Document ID
19760062561
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nakamura, Y.
(Texas Univ. Galveston, TX, United States)
Duennebier, F. K.
(Texas Univ. Galveston, TX, United States)
Latham, G. V.
(Texas Univ. Galveston, TX, United States)
Dorman, H. J.
(Texas, University Galveston, Tex., United States)
Date Acquired
August 8, 2013
Publication Date
September 10, 1976
Publication Information
Publication: Journal of Geophysical Research
Volume: 81
Subject Category
Lunar And Planetary Exploration
Accession Number
76A45527
Funding Number(s)
CONTRACT_GRANT: NAS9-14581
Distribution Limits
Public
Copyright
Other

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